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Table 1:

Radial and rotational velocities for stars in NGC 2682.

No.
ID Vr $\epsilon$ N $V \sin i$ Err $\Delta T$ $P(\chi ^2)$

0003
F 3 32.51 0.63 2 9.3 1.7 736 0.128
0006 F 6 33.77 0.38 2 6.0 2.0 736 0.814
0018 F 18 32.81 0.40 2 11.2 1.4 736 0.775
0020 F 20 33.45 0.31 2 0.9 0.0 734 0.249
0037 F 37 33.11 0.34 2 2.6 2.0 697 0.251
0048 F 48 32.56 0.30 2 0.4 4.4 697 0.688
0054 F 54 34.72 0.36 2 4.6 2.5 734 0.258
0072 F 72 33.17 0.26 2 1.2 2.2 735 0.985
0094 F 94 33.17 0.32 3 8.1 1.4 734 0.796
0096 F 96 33.75 0.34 2 7.3 1.5 695 0.490
0115 F 115 34.24 0.25 3 3.4 2.3 734 0.801
0127 F 127 33.99 0.35 3 5.3 1.6 734 0.193
0157 F 157 32.86 0.36 2 7.3 1.7 694 0.708
0163 F 163 33.06 0.67 2 5.2 1.9 694 0.045
0166 F 166 32.60 0.28 2 2.9 0.0 694 0.944
0193 F 193 33.94 0.26 2 2.6 1.7 694 0.383
0215 F 215 33.08 0.43 2 10.6 1.6 694 0.641
0226 F 226 33.00 0.27 2 2.0 2.0 694 0.860
0227 F 227 33.03 0.31 2 5.0 1.8 694 0.465
0237 F 237 33.52 0.69 2 0.0 0.0 695 0.015
0241 F 241 32.53 0.36 2 5.2 2.1 696 0.409
0243 F 243 33.09 0.36 2 6.4 1.9 696 0.572
0256 F 256 33.24 0.35 2 6.0 3.1 696 0.739
0271 F 271 34.00 0.33 2 4.5 2.2 696 0.976
0272 F 272 30.16 0.56 2 5.5 1.9 696 0.102
0281 F 281 32.74 0.32 2 5.1 1.8 696 0.322
0287 F 287 32.46 0.40 2 8.3 1.7 696 0.424
0289 F 289 33.18 0.50 2 7.3 2.1 697 0.198
0303 F 303 35.12 0.35 2 4.2 2.4 697 0.365
0317 F 317 33.18 0.33 2 2.2 0.0 697 0.744
4018 S 1060 33.58 0.50 1        
7368 S 368 33.82 0.35 2 0.5 3.4 698 0.902
7489 S 489 33.42 0.51 2 8.8 2.2 699 0.829
7657 S 657 32.57 0.32 2 5.7 1.7 699 0.707
7859 S 859 32.07 0.45 2 0.9 3.1 699 0.191
7871 S 871 32.75 0.38 2 5.7 2.2 699 0.580
8524 S 1524 33.04 0.57 1 1.5 4.3    
8639 S 1639 32.90 0.37 2 3.8 0.0 698 0.777
8713 S 1713 32.87 0.64 2 4.2 1.9 698 0.031
8792 S 1792 33.67 0.36 2 3.5 2.2 698 0.436
Note: the star designation corresponds to that used in WEBDA. In the column ID, F refers to Fagerholm (1906) and S to Sanders (1977). The successive columns give: the radial velocity (Vr) and error on the mean ($\epsilon$), the number of measurements (N), the rotation ($V \sin i$) and its error (Err), the time interval covered by the observations ($\Delta T$) and the probability that the scatter is due to random noise ($P(\chi ^2)$).

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